Limits to the Sub-millimetre Isotropic Background

Bibcode
1972Natur.237..154B
DOI
10.1038/237154a0
Beckman, J. E.; Ade, P. A. R.; Huizinga, J. S.; Robson, E. I.; Vickers, D. G.
Referencia bibliográfica

Nature, Volume 237, Issue 5351, pp. 154-157 (1972).

Fecha de publicación:
5
1972
Revista
Nature
Número de autores
5
Número de autores del IAC
0
Número de citas
9
Número de citas referidas
7
Descripción
A PHASE-MODULATED Michelson interferometer1 and a helium cooled Rollin2 photoconductive far infrared detector, at the focus of a 35 cm aperture Cassegrain telescope, were flown at a height of 12.1 km from the Royal Aircraft Establishment, Farnborough, in a Comet 2E aircraft, on November 11, 12 and 16, 1971. The emission spectrum of the stratosphere was obtained in the wavenumber range from 36 cm-1 to 5 cm-1 (wavelengths 280 µm to 2 mm)3. Here we describe an analysis of a portion of this spectrum for features produced by sources outside the Earth's atmosphere.
Tipo
Con árbitro

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